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researcher

P. Evans

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.SR1
same name
  • P. Evans — 17 papers, h 41
  • P. Evans — 17 papers, h 23
  • P. Evans — 12 papers, h 30
  • P. Evans — 12 papers, h 22
  • P. Evans — 3 papers, h 13
  • P. Evans — 2 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedThe SMC X-ray binary SXP4.78 : a new Type II outburst and the identification and study of the optical counterpart

8 citations · 15 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2020★ 7 cited

Optical and X-ray study of the peculiar high mass X-ray binary XMMU J010331.7-730144

Itumeleng M. Monageng, Malcolm J. Coe, David A. H. Buckley +6

For a long time XMMU J010331.7-730144 was proposed as a high-mass X-ray binary candidate based on its X-ray properties, however, its optical behaviour was unclear - in particular p…

astro-ph.HE2019

An X-ray and optical study of the outbursting behaviour of the SMC Be X-ray binary SXP 91.1

Itumeleng Monageng, Malcolm Coe, Jamie Kennea +6

In this paper we report on the optical and X-ray behaviour of the Be X-ray binary, SXP 91.1, during a recent type I outburst. We monitored the outburst using the Neil Gehrels Swift…

astro-ph.HE2019★ 8 cited

The SMC X-ray binary SXP4.78 : a new Type II outburst and the identification and study of the optical counterpart

Itumeleng Monageng, Malcolm Coe, Lee Townsend +6

SXP4.78 was originally discovered in 2000 as a pulsar in the Small Magellanic Cloud (SMC) by the Rossi X-ray Timing Explorer (RXTE) but it was not spatially located at that time. A…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.